The shape of the sodium D lines in a high-temperature helium atmosphere

Details The shape of the sodium D lines in a high-temperature helium atmosphere The shape of the sodium D lines in a high-temperature helium atmosphere

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jphb....8..852e&link_type=abstract

Journal of Physics, Part B - Atomic and Molecular Physics, vol. 8, Apr. 21, 1975, p. 852-863.

Physics

17

Absorption Spectra, D Lines, Helium, High Temperature Gases, Spectral Line Width, Atmospheric Temperature, Compressed Gas, Gas Pressure, Optical Resonance, Sodium, Space Environment Simulation, Stellar Atmospheres

Scientific paper

An experiment was performed to measure the shape of the sodium resonance
doublet (lambda 5890, lambda 5896) in a high-temperature helium
atmosphere. A piston compressor was used to produce temperatures in the
range 3000 K to 5500 K. Absorption-line widths and shifts are reported
and the widths agree well with calculations.

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